Changes between Version 88 and Version 89 of SavinGroup/MergedBeams
- Timestamp:
- 10/07/09 15:57:07 (17 years ago)
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SavinGroup/MergedBeams
v88 v89 4 4 We are measuring rate coefficients of the reaction H^^-^^ + H = H,,2,, . This is an important mechanism for forming H,,2,, molecules which act as a coolant in primordial clouds. This cooling effect is necessary in the formation of the first stars. 5 5 [[br]] 6 ` `[[Image(https://docs.astro.columbia.edu/attachment/wiki/SavinGroup/MergedBeams/First Star.png?format=raw, 50%)]]6 ` `[[Image(https://docs.astro.columbia.edu/attachment/wiki/SavinGroup/MergedBeams/First Star.png?format=raw, 50%)]] 7 7 [[br]] 8 8 [[br]]
